The formation of the first supermassive black holes is one of the
main open questions in our understanding of high-redshift structure
formation. In this book, we aim to provide a summary of
state-of-the-art modern research on this topic, exploring the
formation of massive black holes from a fluid-dynamical,
stellar-dynamical and chemical perspective. The book thus presents
a solid theoretical foundation, a comparison with current
observations and future observational perspectives with upcoming
missions such as the Square Kilometre Array, the European Extremely
Large Telescope, the Euclid satellite as well as possible
detections via gravitational waves.
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